Design of a low noise, wide band, active dipole antenna for a cosmic ray radiodetection experiment
classification
🌌 astro-ph.IM
physics.ins-det
keywords
antennadipoleactivecosmicexperimentnoisewideband
Add this Pith Number to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{OLFNEO6B}
Prints a linked pith:OLFNEO6B badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
An active dipole antenna has been designed to measure transient electric field induced by ultra high energy cosmic rays for the CODALEMA experiment. The main requirements for this detector, composed of a low noise preamplifier placed close to a dipole antenna, are a wide bandwidth ranging from 100 kHz to 100 MHz and a good sensitivity on the whole spectrum.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.